Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars

The late-time integrated Sachs-Wolfe (ISW) imprint of R greater than or similar to 100 h(-1 )Mpc superstructures is sourced by evolving large-scale potentials due to a dominant dark energy component in the ACDM model. The aspect that makes the ISW effect distinctly interesting is the repeated observation of stronger-than-expected imprints from supervoids at z less than or similar to 0.9. Here we analyse the un-probed key redshift range 0.8 < z < 2.2 where the ISW signal is expected to fade in Lambda CDM, due to a weakening dark energy component, and eventually become consistent with zero in the matter dominated epoch. On the contrary, alternative cosmological models, proposed to explain the excess low-z ISW signals, predicted a sign-change in the ISW effect at z approximate to 1.5 due to the possible growth of large-scale potentials that is absent in the standard model. To discriminate, we estimated the high-z Lambda CDM ISW signal using the Millennium XXL mock catalogue, and compared it to our measurements from about 800 supervoids identified in the eBOSS DR16 quasar catalogue. At 0.8 < z < 1.2, we found an excess ISW signal with A(ISW) approximate to 3.6 +/- 2.1 amplitude. The signal is then consistent with the Lambda CDM expectation (A(ISW) = 1) at 1.2 < z < 1.5 where the standard and alternative models predict similar amplitudes. Most interestingly, we also observed an opposite-sign ISW signal at 1.5 < z < 2.2 that is in 2.7 sigma tension with the Lambda CDM prediction. Taken at face value, these recurring hints for ISW anomalies suggest an alternative growth rate of structure in low-density environments at similar to 100 h(-1) Mpc scales.